Beyond HDF - Searching for Early Star Formation in the Infrared

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The success of the Hubble Deep Field (HDF) data in identifying galaxies at redshifts up to ~3 has been quite spectacular. It is possible to extend this to even higher redshifts using infrared techniques, several of which are briefly described in this paper.
3 pages, LaTeX, no figures, uses World Scientific Press style file. To appear in the proceedings from the 18th Texas Symposium (1996)

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